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Star Analyser 200 User Manual

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Star Analyser 200 User Manual PATON HAWKSLEY EDUCATION LTD STAR ANALYSER 200 USER MANUAL v1.2 27th Jan 2014 CONTENTS INSTRUCTIONS Description Care and maintenance A quick look Mounting the Star Analyser 200 First light Troubleshooting Processing Wavelength Calibration Displaying the results graphically Tips for recording spectra of faint objects Visual Use Further advice and information FREQUENTLY ASKED QUESTIONS APPENDIX I BRIGHT STAR SPECTRAL TYPES APPENDIX II TWENTY BRIGHTEST WOLF RAYET STARS APPENDIX III TELLURIC LINES (O2) APPENDIX IV HYDROGEN BALMER LINES APPENDIX V “INTRODUCING THE STAR ANALYSER 200” STAR ANALYSER 200 INSTRUCTIONS Description The Star Analyser 200 is a high efficiency 200 lines/mm transmission diffraction grating, blazed in the first order. It is mounted in a low profile 1.25 inch diameter threaded cell, to be compatible with most telescopes and accessories. It has been designed to make the production of low resolution spectrum images of a wide range of point like astronomical objects as easy as possible. It complements a wide range of types of camera used in astro-imaging. It can however also be adapted for visual use. It is designed primarily for applications where it is difficult to achieve the optimum spacing needed for the Star Analyser 100. The SA200 gives the same length of spectrum when mounted half the distance from the camera sensor compared with the SA100 (Note that where there is sufficient space to achieve the optimum spacing, the SA100 model is the recommended option) Typical applications of the SA200 are: Mounting in close coupled filter wheels (The smaller distance requirement, low profile design and optional mounting kit allow the SA200 to be accommodated in a wider range of filter wheels than the SA100) With larger aperture, longer focal length telescopes used with larger camera sensors where a longer spectrum can be produced using the SA200 to give optimum resolution. See also Appendix V “Introducing the Star Analyser 200” for further technical information on the SA200 Care and maintenance The Star Analyser has been designed and built to give many years of trouble free service. It cannot be dismantled by the user. To protect the delicate diffraction grating surface, it has been sealed between anti-reflection coated glass cover discs. The sealed unit is fixed in the cell in the correct alignment. As with any optical device, care should be taken to protect the optical surfaces. It should be stored in its protective box when not in use. (After use, any dew which may have condensed on the device should be allowed to evaporate before closing the box) Avoid touching the glass. Any dust should be removed with a blower brush or clean oil free canned air. More stubborn marks and fingerprints can be removed with care using conventional lens cleaning techniques. (Lens cleaning fluids should be used very sparingly to avoid the risk of seepage of the fluid between the glass elements) A quick look If you hold the Star Analyser up to you eye and view a compact source of white light through it, you will see the light source flanked by a series of rainbow spectra, stretching away in both directions. One of the pair of spectra closest to the light source will look significantly brighter than the others. This is the blazed first order spectrum and is the one we are aiming to image, along with the straight through view of the light source (the zero order) If you look at the edge of the filter cell, you will see a white line marking the direction of the blazed first order. This The blazed first order spectrum will help identify the right spectrum and line it up in dominates the other orders in this the field of view of your camera. view of a low energy light bulb. Mounting the Star Analyser 200 General The SA200 uses a standard 1.25 inch filter cell design and is mounted between the telescope and camera at the recommended distance from the camera sensor using standard adapters. (See FAQ 13 and 14 to calculate the recommended distance for your particular setup) Orientate the grating so the direction indicated by the white mark is on the horizontal axis of the camera and to the right as you view from behind the camera. Mounting in filter wheels The SA200-F has a significantly lower profile than the SA100 (7.7mm total height including thread compared with 11.2mm for the SA100) which allows it to be mounted in filter wheels designed for 1.25 inch filters without risk of fouling the wheel housing. (Note that the low profile design means that, unlike the SA100, there is no thread available above the grating to screw on other accessories.) The SA200-F can be aligned with the camera sensor and held in the correct orientation for example with PTFE tape on the thread or a spot of hot melt adhesive. Provided there is sufficient clearance, the SA200-F can also be mounted in wheels designed to take unmounted drop in filters. An optional mounting kit for this purpose, consisting of a carrier plate, spacers and an internally threaded collar to fix the SA200 in position in the plate is available from Paton Hawksley The pre-punched 1mm thick black styrene carrier plate is trimmed to size using a craft knife (score and snap) or scissors to match the filter size used in the wheel (eg 50mm square, 2 inches round etc) and the SA200 mounted through the pre punched hole, orientated and fixed in position using the threaded collar. Additional spacers of the same material, supplied pre-punched with oversized holes can be added above or below the carrier plate as required to increase the total thickness and place the SA200 at the optimum height to clear the wheel housing. It is even feasible to fabricate a carrier which lowers the position of the SA200 below that shown here if necessary, by laminating the material (bonded using polystyrene cement). As a result, provided a clearance of at least 7.7mm (The total height of the SA200) is available within the filter wheel it should be possible to fabricate a suitable carrier. Users are advised to check their particular model of filter wheel to ensure there is enough clearance. Tip:- To ensure a good fit when trimming the plates to size, first make a template using backed label paper and check it fits correctly in the filter wheel. Then stick the label centrally onto the plate and trim round it. A similar technique can also be used to mount the SA200-F in a (user supplied) blank 2 inch filter cell for wheels designed for 2 inch screw in filters. (Note that, since the light cone from the star is only dispersed into a spectrum beyond the grating, any vignetting of the field due to the smaller aperture of the SA200, compared with filters used for imaging, is not a problem provided the zero order image of the star is placed within the unvignetted area.) First light Delta Virginis (type M) Vega (type A) Set your telescope and camera up on a bright star and centre it in the field. Spectral type M stars are a good first target as they show nice broad spectrum lines which are easy to see. Alternatively type A stars show narrow dark absorption lines due to Hydrogen. You can see a list of the spectral types of all bright stars down to mag +2.5 in Appendix I Mount the Star Analyser in front of your camera, orientating it so the direction indicated by the white mark is on the horizontal axis of the camera and to the right as you view from behind the camera. You should still be able to see the image of the star but it will be somewhat fainter. (Adjust to bring the star back into focus). Move the telescope slightly so that the star image is on the left edge of the frame. You should then see the spectrum of the star spread out horizontally across the field, with increasing wavelength (blue to red) running from left to right. (Note that because the light from the star is now spread out over many more pixels, you may have to increase the exposure to see the spectrum clearly. You should now be able to see some lines in the spectrum. If not, adjust the camera settings and focus slightly until you get the sharpest, clearest spectrum. Congratulations! You have recorded your first spectrum with the Star Analyser. Troubleshooting The spectrum seems very faint. Are you sure you have found the right spectrum? Move the telescope until the star image is on the right of the field. You should just be able to see a faint spectrum running from right to left. It should be much fainter than the spectrum on the other side of the star image. If it is brighter, rotate the Star Analyser through 180 degrees. The spectrum is too long to fit across the field. (Take care not to confuse the infra red end of the wanted spectrum with the blue end of the next order spectrum which will be much fainter but will overlap.) This is because the dispersion (The amount by which the light of given wavelength is deflected) is too high. The SA200 is designed to work at half the distance from the camera compared with the SA100. If you cannot mount the SA200 close enough to the camera sensor to fit the spectrum and star image in the field it is recommended that you use the Star Analyser 100 instead The spectrum is rather short You can increase the length of the spectrum by increasing the grating to sensor distance.
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